First Direct Measurement of an Astrophysical p-Process Reaction Cross Section Using a Radioactive Ion Beam

We have performed the first direct measurement of the ^83Rb (p, γ) radiative capture reaction cross section in inverse kinematics using a radioactive beam of ^83Rb at incident energies of 2. 4 and 2. 7A MeV. The measured cross section at an effective relative kinetic energy of E₂₌=2. 393 MeV, which lies within the relevant energy window for core collapse supernovae, is smaller than the prediction of statistical model calculations. This leads to the abundance of ^84Sr produced in the astrophysical p process being higher than previously calculated. Moreover, the discrepancy of the present data with theoretical predictions indicates that further experimental investigation of p-process reactions involving unstable projectiles is clearly warranted.